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Integration of differential wavefront sampling with merit function regression for efficient alignment of three-mirror anastigmat optical system

机译:差分波前采样与优点函数回归相集成,可有效对准三反射镜的光学系统

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摘要

We first studied the characteristics of alignment performances of two computer-aided alignment algorithms i.e. merit function regression (MFR) and differential wavefront sampling (DWS). The initial study shows i) that, utilizing damped least square algorithm, MFR offers accurate alignment estimation to the optical systems with non-linear wavefront sensitivity to changes in alignment parameters, but at the expense of neglecting the coupling effects among multiple optical components, and ii) that DWS can estimate the alignment state while taking the inter-element coupling effects into consideration, but at the expense of increased sensitivity to measurement error associated with experiment apparatus. Following the aforementioned study, we report a new improved alignment computation technique benefitted from modified MFR computation incorporating the concept of standard DWS method. The optical system used in this study is a three-mirror anastignmat (TMA) based optical design for the next generation geostationary ocean color instrument (GOCI-II). Using an aspheric primary mirror of 210 mm in diameter, the F/7.3 TMA design offers good imaging performance such as 80% in 4 um in GEE, MTF of 0.65 at 65.02 in Nyquist frequency. The optical system is designed to be packaged into a compact dimension of 0.25m * 0.55m x 1.050m. The trial simulation runs demonstrate that this integrated alignment method show much better alignment estimation accuracies than those of standard MFR and DWS methods, especially when in presence of measurement errors. The underlying concept, computational details and trial simulation results are presented together with implications to potential applications.
机译:我们首先研究了两种计算机辅助对准算法的对准性能的特征,即优点函数回归(MFR)和差分波前采样(DWS)。初步研究表明:i)利用阻尼最小二乘算法,MFR可以为光学系统提供精确的对准估计,而非线性系统对对准参数的变化具有非线性波前灵敏度,但会忽略多个光学组件之间的耦合效应,并且ii)DWS可以在考虑元素间耦合效应的同时估算对准状态,但要以增加对与实验设备相关的测量误差的敏感性为代价。继前述研究之后,我们报告了一种新的改进的对齐计算技术,该技术得益于结合标准DWS方法概念的改进的MFR计算。这项研究中使用的光学系统是基于三镜面Anastignmat(TMA)的光学设计,用于下一代地球静止海洋彩色仪器(GOCI-II)。 F / 7.3 TMA设计使用直径为210 mm的非球面主镜,可提供良好的成像性能,例如在4 um的GEE中为80%,在Nyquist频率为65.02时的MTF为0.65。光学系统的设计尺寸为0.25m * 0.55m x 1.050m。模拟试验表明,这种集成的对准方法比标准MFR和DWS方法具有更好的对准估计准确性,尤其是在存在测量误差的情况下。介绍了基本概念,计算细节和试验仿真结果以及对潜在应用程序的含义。

著录项

  • 来源
  • 会议地点 San Diego CA(US)
  • 作者单位

    Space Optics Laboratory, Dept. of Astronomy, Yonsei University / Korea, Republic of Institute of Space Science and Technology, Yonsei University / Korea, Republic of;

    Korea Aerospace Research Institute / Korea, Republic of;

    Dept. of Science of Measurement, University of Science Technology / Korea, Republic of Korea Research Institute of Standards and Science / Korea, Republic of;

    McDonald Observatory, The University of Texas at Austin, 1 University Station C1402, Austin, TX78712/United States;

    Space Optics Laboratory, Dept. of Astronomy, Yonsei University / Korea, Republic of Institute of Space Science and Technology, Yonsei University / Korea, Republic of;

    Dept. of Science of Measurement, University of Science Technology / Korea, Republic of Korea Research Institute of Standards and Science / Korea, Republic of;

  • 会议组织
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 应用光学;
  • 关键词

    Alignment; Merit function regression; Differential wavefront sampling; Zernike polynomial; Three mirror;

    机译:对准;优点函数回归;差分波前采样;泽尼克多项式;三面镜;

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